activity
20032017
most citedHerschel Measurements of Molecular Oxygen in Orion

170 citations · 934 across the 17 of their papers we have counts for

collaborators

17 papers

astro-ph.GA2017★ 3 cited

Odin observations of ammonia in the Sgr A +50 km/s Cloud and Circumnuclear Disk

Aa. Sandqvist, Å. Hjalmarson, U. Frisk +4

Context. The Odin satellite is now into its sixteenth year of operation, much surpassing its design life of two years. One of the sources which Odin has observed in great detail is…

astro-ph.EP2016★ 103 cited

Isotopic ratios of H, C, N, O, and S in comets C/2012 F6 (Lemmon) and C/2014 Q2 (Lovejoy)

N. Biver, R. Moreno, D. Bockelée-Morvan +15

The apparition of bright comets C/2012 F6 (Lemmon) and C/2014 Q2 (Lovejoy) in March-April 2013 and January 2015, combined with the improved observational capabilities of submillime…

astro-ph.SR2015★ 16 cited

On the accretion process in a high-mass star forming region - A multitransitional THz Herschel-HIFI study of ammonia toward G34.26+0.15

M. Hajigholi, C. M. Persson, E. S. Wirström +8

[Abridged] Our aim is to explore the gas dynamics and the accretion process in the early phase of high-mass star formation. The inward motion of molecular gas in the massive star f…

astro-ph.GA2014★ 46 cited

Herschel HIFI observations of O toward Orion: special conditions for shock enhanced emission

Jo-Hsin Chen, Paul F. Goldsmith, Serena Viti +18

We report observations of molecular oxygen (O) rotational transitions at 487 GHz, 774 GHz, and 1121 GHz toward Orion Peak A. The O2 lines at 487 GHz and 774 GHz are detected at…

astro-ph.GA2014★ 18 cited

Upper limits to interstellar NH+ and para-NH2- abundances. Herschel-HIFI observations towards Sgr B2 (M) and G10.6-0.4 (W31C)

C. M. Persson, M. Hajigholi, G. E. Hassel +12

The understanding of interstellar nitrogen chemistry has improved significantly with recent results from the Herschel Space Observatory. To set even better constraints, we report h…

astro-ph.GA2013

Hydroxyl, water, ammonia, carbon monoxide and neutral carbon towards the Sgr A complex

Roland Karlsson, Aage Sandqvist, Åke Hjalmarson +4

We observed OH, HO, HN, CO, and C towards the +50 km/s cloud (M-0.02-0.07), the CND and the +20 km/s (M-0.13-0.08) cloud in the Sgr A complex with the VLA, Odin…